CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.

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George Mason University (USA) - University of Michigan (USA) - University of Cambridge (UK)

CHIANTI consists of a critically evaluated set of up-to-date atomic data, together with user-friendly programs written in Interactive Data Language (IDL) and Python to calculate the spectra from astrophysical plasmas.

The CHIANTI package is freely available.
If you use the package, we only ask you to appropriately acknowledge CHIANTI .

- The Chianti wine-producing area of Tuscany, Italy -

CHIANTI Version 7 released

We would like to announce the release of version 7.0 of the CHIANTI database for astrophysical spectroscopy. With Version 7.0, CHIANTI now includes data for several new ions as well as significant updates to many ions, including several key Fe species routinely observed by Hinode/EIS and SDO. Also, a completely new implementation of the CHIANTI software in the Python programming language has been developed and is freely available on the web (ChiantiPy).

We are grateful to individual scientists and funding agencies for their support.